New constraints on the magnetization of the cosmic web using LOFAR Faraday rotation observations
Artikel i vetenskaplig tidskrift, 2020

Measuring the properties of extragalactic magnetic fields through the effect of Faraday rotation provides a means to understand the origin and evolution of cosmic magnetism. Here we use data from the LOFAR Two-Metre Sky Survey (LoTSS) to calculate the Faraday rotation measure (RM) of close pairs of extragalactic radio sources. By considering the RM difference (Delta RM) between physical pairs (e.g. double-lobed radio galaxies) and non-physical pairs (i.e. close projected sources on the sky), we statistically isolate the contribution of extragalactic magnetic fields to Delta RM along the line of sight between non-physical pairs. From our analysis, we find no significant difference between the ?RM distributions of the physical and non-physical pairs, limiting the excess Faraday rotation contribution to <1.9 rad/m(2) (similar to 95% confidence). We use this limit with a simple model of an inhomogeneous universe to place an upper limit of 4 nG on the cosmological co-moving magnetic field strength on Mpc scales. We also compare the RM data with a more realistic suite of cosmological MHD simulations, that explore different magnetogenesis scenarios. Both magnetization of the large scale structure by astrophysical processes such as galactic and AGN outflows, and simple primordial scenarios with seed magnetic field strengths <0.5 nG cannot be rejected by the current data; while stronger primordial fields or models with dynamo amplification in filaments are disfavoured.

radio continuum: galaxies

galaxies: magnetic fields

galaxies: active

large:scale structure of Universe

techniques: polarirnetnc

Författare

S. P. O'Sullivan

Dublin City University

Universität Hamburg

M. Bruggen

Universität Hamburg

F. Vazza

Universität Hamburg

Istituto nazionale di astrofisica (INAF)

Universita di Bologna

E. Carretti

Istituto nazionale di astrofisica (INAF)

N. Locatelli

Istituto nazionale di astrofisica (INAF)

Universita di Bologna

C. Stuardi

Universita di Bologna

Istituto nazionale di astrofisica (INAF)

V. Vacca

INAF Osservatorio Astron Cagliari

T. Vernstrom

CSIRO Astronomy and Space Science

G. Heald

CSIRO Astronomy and Space Science

Cathy Horellou

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik, Extragalaktisk astrofysik

T. W. Shimwell

Netherlands Institute for Radio Astronomy (ASTRON)

Universiteit Leiden

M. J. Hardcastle

University of Hertfordshire

C. Tasse

Université PSL

H. Rottgering

Universiteit Leiden

Monthly Notices of the Royal Astronomical Society

0035-8711 (ISSN) 1365-2966 (eISSN)

Vol. 495 3 2607-2619

Ämneskategorier

Astronomi, astrofysik och kosmologi

Annan fysik

Fusion, plasma och rymdfysik

DOI

10.1093/mnras/staa1395

Mer information

Senast uppdaterat

2020-09-03